Discovery of radio emission from X-ray pulsar PSR J1852+0040

Details Discovery of radio emission from X-ray pulsar PSR J1852+0040 Discovery of radio emission from X-ray pulsar PSR J1852+0040

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..501....1m&link_type=abstract

The Astronomer's Telegram, #501

Astronomy and Astrophysics

Astronomy

3

Radio, X-Ray, Neutron Stars, Pulsars, Supernova Remnants, Transients

Scientific paper

We report the detection of radio pulses from X-ray pulsar J1852 +0040 with the same period (105 ms) at frequency 111.23 MHz. This pulsar was discovered in March 2005 by Gotthelf et al. (astro-ph/0503424) in the compact central object (CCO) of the young supernova remnant Kes 79 using XMM-Newton observations. Our observations were made during 24 days in April-May 2005 using the Large Phased Array in Pushchino Radio Astronomy Observatory (PRAO, Russia), sensitive transit radio telescope consisting of 16384 dipoles and on operating frequency of 110.5 +/- 1.5 MHz.

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